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Fig. 1


3 mm continuum emission (in gray contours) on top of an HST ACS F435W filter gray-scale image to facilitate a comparison of the location and distribution of the emission with respect to the dust lanes at the center of NGC 1614. This image of the 3 mm continuum emission was created using uniform weighting, which resulted in a sensitivity of 1σ = 59.8 μJy beam-1. The contours start at 3σ and are spaced in steps of 5σ. The cross marks the phase center of the observations, placed at the center of the molecular gas ring. The beam (see also Table 1) is shown in the lower right corner. North is up, east to the left.

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